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  4. Combination Center

Combination Center

Contribution to ITRF2020

The IDS 16 series is the DORIS contribution to the 2020 realization of the International Terrestrial Reference Frame.

It provides weekly positions of the DORIS stations and daily Earth Orientation Parameters

This series of 1456 weekly SINEX files contains positions of 201 DORIS stations located at 87 DORIS sites from 1993.0 to 2021.0. The series is the combination of ESA 13 (ESA/ESOC), GOP 67 (Geodetic Observatory Pecny) , GRG 43 (CNES/CLS) and GSC 51 (NASA/GSFC) DORIS multi-satellite solutions processed for the realization of the ITRF2020 according to the IDS standards.

 

DOI and Metadata

This product is referenced with a DOI: 10.24400/312072/i01-2021.001

More metadata

 

Product access

The product (zipped SINEX files idsyydddwd16.snx.Z*) can be freely downloaded at the CDDIS HTTPS server or via the non authenticated IGN FTP site (the FTP protocol may not be supported by your browser, the alternative is to use a FTP client such as WinSCP, FileZilla, MobaXterm ). 

*naming convention

 

Citation

If you use the data, please cite: "The IDS 16 series was produced by the IDS Combination Center (DOI: 10.24400/312072/i01-2021.001)"

 

Contacts

For any technical issues or additional information related to the IDS 16 series, users are advised to contact the Combination Center

 

Acknowledgement

The work of the Combination Center is supported by CNES.

 

References

Moreaux, G.; Lemoine, F.G.; Capdeville, H.; Otten, M.; Štěpánek, P.; Saunier, J.; Ferrage, P., 2022. The international DORIS service contribution to ITRF2020, ADVANCES IN SPACE RESEARCH, DOI: 10.1016/j.asr.2022.07.012 OPEN ACCESS

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Last Updated: 17 October 2024

The pages of the Combination Center provide information about the activity and products of the Combination Center of the International DORIS Service (IDS). They are mainly of interest to the IDS Analysis Centers as well as to other other users, including mission flight times with responsibilities for precise orbit determination.

Horizontal displacement of the DORIS stations, reflecting the plate tectonique motion (Credits CNES/CLS/IDS) 

Horizontal displacement of the DORIS stations, reflecting the plate tectonique motion (Credits CNES/CLS/IDS)
Reference: Moreaux et al. (2016)

 

Activity of the Combination Center

Currently, six IDS Analysis Centers (ESA, GOP, GRG, GSC, IGN and INA) provide direct input for the official IDS products (station coordinates and Earth Orientation Parameters - EOPs). In addition, after the success of the pilot project to deliver an IDS combined solution for the ITRF2008 realization, the IDS decided to extend the combination process to an operational service. Thus, since 2010, the IDS Combination Center (CC) routinely evaluates the IDS AC station position and EOPs series and combines it to form the official IDS combined solution. The IDS CC is also in charge of the generation of all the DORIS coordinate time series from all the IDS AC (in addition to the IDS CC) SINEX series.

Since the realization of the ITRF2014, the IDS CC is responsible for the elaboration and update of the DPOD solution, i.e. DORIS station positions and velocities for the Precise Orbit Determination (POD) of the DORIS satellites.

All the computations realized by the IDS Combination Center are based on the IGN CATREF (Combination and Analysis of Terrestrial Reference Frames) package (Altamimi et al., 2002).

 

The Products

Weekly solutions

Every three months (with a latency of three months), the six IDS ACs submit SINEX solutions including weekly station positions, daily EOPs and the full covariance matrix. After evaluation by the IDS Combination Center, these solutions are combined in a standard least-squares adjustment to form the IDS weekly combined solutions.

The evaluation of the IDS AC solution consists of monitoring the similarity transformation parameters (the Helmert parameters) of the series with respect to the current ITRF realization as well as of analyzing the EOP differences with the IERS C04 series. The Helmert parameters, global station position 3D weighted residuals and EOP differences can be visualized through the IDS web service.

 

Station Coordinate Time series

After alignment of the weekly SINEX files on the current ITRF, for all the ACs and all the DORIS stations, the IDS CC generates the coordinate time series. These time series are stored in the  STCD files to be downloaded from the IDS Data Centers. Note that these coordinate time series can also be visualized from the IDS web service (see for exemple the time series for Toulouse). 

 

Cumulative solution

Besides the weekly combined solutions, a long-term DORIS position and velocity cumulative solution is updated and released every three months. In that solution, a piecewise linear (position+velocity) model is used to describe the station motions. The cumulative position and velocity solution is obtained from the stacking of the weekly solution files and is then aligned to the current ITRF. The residuals of this stacking are of particular interest since they depict non-linear station motions.

 

DORIS extension of the ITRF for Precise Orbit Determination (DPOD)

From the DORIS cumulative solution, the IDS CC generates the DPOD solution. This solution contains positions and velocities of all the DORIS tracking stations for Precise Orbit Determination (POD) applications. It differs from the cumulative solutions by (1) it also includes position and velocity of the newest DORIS stations which were not already observed by the IDS ACs and, (2) between two successive DPOD solutions, for all the stations, we only update the positions if the new ones significantly differ from the previous ones.

 

DORIS Sinex master file

To facilitate the access to the geographic positions of all the DORIS stations, the IDS has created a new IDS product: the DORIS SINEX Master file.
In addition to the geographic positions, that file also contains for each DORIS station information (type and eccentricity) of the antennas in SINEX format. That file, maintained by the IDS Combination Center, is available from the IDS Central Bureau ftp site

 

Product names

Network products

  • dpod2014_vx.y.snx.Z: DPOD solution (“x.y” denotes the version number).

  • dpod2014_vx.y.txt.Z: DPOD solution without covariance matrix.

  • idsyydxx.snx.Z: cumulative solution (“yy” denotes the year of submission and “xx” stands for the series number).

  • idsyydddwdxx.snx.Z: weekly combined solution (“yy” stands for the last two digits of year of the first observation, “ddd” for three-digit day of year of the first observation, and “xx” for the series number).

One-station products

  • idsyywdxx.stcd.aaaa.Z: time series of station coordinates (“yy” denotes the year of submission, “xx” stands for the series number, and “aaaa” denotes the four-character station acronym).

  • idsyywdxx.stcd.aaaa.gif: plot of time series of station coordinates.

 

Archive

These official products are available at the IDS Data Centers, CDDIS and IGN (alternate link)

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Last Updated: 15 January 2019

DPOD: DORIS extension of the ITRF for Precise Orbit Determination

The so-called DPOD product is a set of coordinates and velocities of all the DORIS tracking stations for Precise Orbit Determination (POD) applications

 

DPOD2020

The computation of the DPOD2020 solutions is realized by the IDS Combination Center (CC).

The set of coordinates/velocities herein is the result of a three-step process:

  1. Computation of a DORIS position and velocity cumulative solution from the latest IDS combined series since 1993.0.
  2. Addition of the newest DORIS stations not already in the IDS combined series from the DORIS mails.
  3. Validation:
    • IDS CC internal validation (including position and velocity differences wrt ITRF2020, previous release…).
    • Orbit validation by Frank Lemoine (NASA), Alexandre Couhert (CNES), John Moyard (CNES) and Nikita Zelensky (UMD).

The positions and velocities are given at epoch 2000.0.

The DPOD2020 solutions are available in both SINEX (.snx; description) and text (.txt; description given in header of product files) formats. 

Since version 2.0, the DPOD2020 solutions provide, in addition to the usual/classical station positions and velocities, annual and semi-annual station position corrections as well as post-seismic deformation corrections. Seasonal and post-seismic deformation corrections are given in ASCII text files: dpod2020_020_freq_corr.txt and dpod2020_020_psd_corr.txt, respectively.

 

Citation:

Moreaux, G.; Lemoine, F.G.; Zelensky, N.P.; Moyard, J.; Couhert, A., 2023. DPOD2020: a DORIS extension of the ITRF2020 for Precise Orbit Determination, ADVANCES IN SPACE RESEARCH, 72(11):4625-4650, DOI : 10.1016/j.asr.2023.10.006 OPEN ACCESS

 

DPOD2020 releases available at CDDIS (https) and IGN (ftp):

  • January 2023 – version #1 - dpod2020_01 - technical report
  • February 2024 - version #2 - dpod2020_02 - technical report (for more details on POD tests, see AGU Fall 2023 presentation) 
  • December 2024 - version #3 - dpod2020_03 - technical report

 

DPOD2014

The computation of the DPOD2014 solutions by the IDS Combination Center (CC) started in 2016.

The set of coordinates/velocities herein is the result of a five-step process:

  1. Computation of a DORIS position and velocity cumulative solution from the latest IDS combined series.
  2. From the previous DPOD2014 version, update of positions and velocities for the DORIS stations showing coordinate (resp. velocity) differences larger than XX mm (resp. YY mm/yr).
  3. Addition of the DORIS stations with observations before 1992 from DPOD2008 v1.14 (after alignment to ITRF2014).
  4. Addition of the newest DORIS stations not already in the IDS combined series from the DORIS mails.
  5. Validation:
    • IDS CC internal validation (including position and velocity differences wrt ITRF2014, previous release…).
    • Orbit validation by Pascal Willis (IGN), Frank Lemoine (NASA), Alexandre Couhert (CNES) and Nikita Zelensky (SGT).

The positions and velocities are given at epoch 2000.0.

The DPOD2014 solutions are available in both SINEX (.snx; description) and text (.txt; description given in header of product files) formats. 

 

Citation:

Moreaux, G.; Willis, P.; Lemoine, F.G.; Zelensky, N.P.; Couhert, A.; Ait Lakbir, H.; Ferrage, P., 2019. DPOD2014: a new DORIS extension of ITRF2014 for Precise Orbit Determination, ADVANCES IN SPACE RESEARCH, 63(1):118-138, DOI : 10.1016/j.asr.2018.08.043

Network of DPOD2014 v05

 

DPOD2014 releases available at CDDIS and IGN:

  • March 2017 – version #1 - dpod2014_01 - technical report
  • October 2017 – version #2 - dpod2014_02 - technical report
  • November 2018 – version #3 - dpod2014_03 - technical report
  • November 2019 – version #4 - dpod2014_04 - technical report
  • August 2020 – version #5 - dpod2014_05 - technical report

 

DPOD2008

DORIS coordinates based on ITRF2008 for POD

  • Product available at CDDIS and IGN
  • Detailled description at IPGP
  • Citation:
  • Willis, P.; Zelensky, N.P.; Ries, J.; Soudarin, L.; Cerri, L.; Moreaux, G.; Lemoine, F.G.; Otten, M.; Argus, D.F.; Heflin, M.B., 2016.
    DPOD2008, a DORIS-oriented Terrestrial Reference Frame for Precise Orbit Determination,
    IAG SYMPOSIA SERIES,143, 175-181, DOI: 10.1007/1345_2015_125

     

    DPOD2005

    DORIS coordinates based on ITRF2005 for POD

    • Product available at CDDIS and IGN
    • Detailled description at IPGP
    • Citation:
    • Willis, P.; Ries, J.C.; Zelensky, N.P.; Soudarin, L.; Fagard, H.; Pavlis, E.C.; Lemoine, F.G., 2009.
      DPOD2005 : An extension of ITRF2005 for Precise Orbit Determination,
      ADVANCES IN SPACE RESEARCH, 44(5), 535-544, DOI: 10.1016/j.asr.2009.04.018

       

      DPOD2000

      DORIS coordinates based on ITRF2000 for POD

      • Product available at CDDIS and IGN
      • Citation:
      • Willis, P; Ries, JC. 2005.
        Defining a DORIS core network for Jason-1 Precise Orbit Determination based on ITRF2000, Methods and realizations,
        JOURNAL OF GEODESY 79 (6-7):370-378, DOI:10.1007/s00190-005-0475-9
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      Last Updated: 13 March 2025

      Cumulative solution

      Cumulative solution

      Since the IDS contribution to the realization of the ITRF2014, the IDS Combination Center (CC) routinely (every three months) computes a DORIS position and velocity cumulative solution from the latest IDS combined series. The cumulative solution provides the usual/classical estimates: station positions and velocities at a mean epoch.

      All the details on the elaboration of the IDS cumulative solutions aligned to ITRF2014 can be found in Moreaux et al. (2016).

       

      DORIS horizontal velocities from the IDS combined solution   DORIS vertical velocities from the IDS combined solution

      Figure - ids22d01 and ITRF2020 velocities with formal error smaller than 2.5 mm/yr (left: horizontal; right: vertical).

       

      Releases aligned to ITRF2020:

      • January 2023 – version #1 – Time span: 1993.0-2022.0 – ids22d01 - Product available at CDDIS (HTTPS authenticated) and IGN (FTP link)  Validation results 

      See the residuals on the IDS webservice

       

      Releases aligned to ITRF2014:

      • August 2020 – version #5 – Time span: 1993.0-2020.0 - ids20d05 - Product available at CDDIS and IGN - Validation results - Residuals
      • September 2019 – version #4 – Time span: 1993.0-2019.0 - ids19d04 - Product available at CDDIS and IGN - Validation results - Residuals
      • June 2018 – version #3 – Time span: 1993.0-2018.0 - ids18d03 - Product available at CDDIS and IGN - Validation results - Residuals
      • October 2017 – version #2 – Time span: 1993.0-2017.0 - ids17d02 - Product available at CDDIS and IGN - Validation results - Residuals
      • March 2017 – version #1 – Time span: 1993.0-2016.0 - ids17d01 - Product available at CDDIS and IGN - Validation results - Residuals

       

      Input data:

      • Weekly SINEX files from the latest IDS combined series.
      • Station discontinuities (online file).
      • Tie vectors (online file).

      Output files:

      • Cumulative solution in SINEX format.
      • Station position residuals (online plots).
      • Tie discrepancies (estimated – measured ties; online plot).

      Citation:

      Moreaux, G., Lemoine, F.G., Argus, D.F., Santamaría-Gómez, A., Willis, P., Soudarin, L., Gravelle, M., and Ferrage, P., 2016. Horizontal and vertical velocities derived from the IDS contribution to ITRF2014, and comparisons with geophysical models, Geophysical Journal International, 207(1), 209-227, doi:10.1093/gji/ggw265

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      Last Updated: 13 January 2023

      IDS contribution to the IERS ITRF2008 call for participation

      (First iteration Feb. 2009)

      (Last iteration Nov. 2009)
      The IDS-3 SINEX time series may be downloaded at ftp://ftp.ids-doris.org/pub/ids/combinations/ITRF2008-IDS/IDS-3/

      ITRF2008 Call

      IDS Analysis

      Two IDS Analysis Working Group meetings have been organized in March and June 2008 in Paris, Bureau des Longitudes, and an IDS workshop in Nice, 12-14 November 2008. Eight DORIS analysis centers participated including four official analysis centers (IGN; LCA ; GOP ; ESA), and four candidate analysis centers (NCL - University of Newcastle; GAU - Geoscience Australia; INA - Institute of Astronomy, Russian Academy of Sciences, and GSC - NASA Goddard Space Flight Center). All these centers are working to provide SINEX solutions for inclusion in the IDS combined solution that will be submitted to the IERS for ITRF2008.

      This is an important step for IDS Analysis centers! Indeed for ITRF2005, only two individual DORIS solutions were included: IGN and LCA. A main goal was to improve the models and processing strategies of the new ACs, to discuss the standards and to get ready for the IDS contribution to ITRF2008.


      The IDS Analysis Centers are listed hereafter. Analysis activities are coordinated by F. Lemoine.

      Analysis Center Acron. Contact
      Geodetic Observatory of Pecny, Czech Republic gop Petr Stepanek
      Institute of Astronomy, Russian Academy of Sciences (INASAN), Russia ina Sergey Kuzin
      Surya Tatevian
      CNES/CLS, France lca Laurent Soudarin
      Hugues Capdeville
      Jean-Michel Lemoine
      IGN/IPGP, France ign Pascal Willis
      Marie-Line Gobinddass
      ESA/ESOC, Germany esa Michiel Otten
      Geoscience Australia, Australia
      (with support of GSFC)
      gau Ramesh Govind
      Frank Lemoine
      GSFC, USA gsc Frank Lemoine
      University of Newcastle, UK ncl Philip Moore


      The IDS combinations of weekly solutions for the station coordinates and the Earth Orientation Parameters are realized with CATREF, the IGN/LAREG Software.

      Coordination Center Acron. Contact
      CLS/CNES ids (TBC) JJacques Valette
      Philippe Yaya
      Pascale Ferrage
      LAREG/IGN (software and strategy support) - Zuheir Altamimi

       

      Weekly SINEX series contributions

      The following table summarizes the AC submissions and associated main models as well as the DORIS SINEX series provided for the contribution to ITRF2008.
      See also the DORIS satellites constellation history status.

      AC Software Sol. Id. Type (1) Data span Satellites (2) Earth Gravity
      Field
      Constraint EOPs Desc.
      gop BERNESE 5.0 wd31 var-cov 1999.0-2006.9 Spot 2/4/5
      Topex Envisat
      Jason-1 in 2002
      EIGEN-GL04S annual, 100X100 loose motion, rate dsc
      more
      ina GYPSY/OASIS 4.03 wd03 var-cov 1997.0-2008.8 Spot 2/5
      Spot 4 (except 05/98-01/99)
      Topex Envisat
      GGM01C
      fixed, 120x120
      loose motion
      rate (constrained)
      LOD, UT1
      dsc
      more
      lca GINS/DYNAMO wd20 var-cov 1993.0-1998.4
      1999.4-2002.0
      2002.0-2008.0
      Spot 2/3/4/5
      Topex & Envisat
      (Topex/Envisat orbits with SLR)
      EIGEN_GL04S
      drift, annual
      semi-annual
      95x95
      loose motion dsc
      readme
      more
      ign GYPSY/OASIS 5.0 wd08 var-cov 1993.0-2008.8 Spot 2/3/4/5
      Topex Envisat
      GGM03S
      fixed, 120x120
      loose motion
      rate (constrained)
      LOD, UT1
      dsc
      readme
      more
      gau GEODYN wd06 var-cov 2003.0-2008.8 Spot 2/4/5
      Envisat
      Jason-1
      GGM02C
      annual, 160x160
      loose motion
      UT1
      dsc
      more
      esa NAPEOS wd01 NEQ 1998.0-2008.0 Spot 2/4/5
      Envisat
      (Envisat orbits with SLR)
      EIGEN-GL05C loose motion, rate
      LOD
      dsc
      more

      (1) var-cov: variance-covariance, NEQ: Normal Equation
      (2) Specific recommendation for Jason-1 is to exclude Jason-1 data after 2003 because of the USO sensitivity to SAA (cf AWG-June 2008)

       

      Compliancy with IERS Call

      The delivered SINEX are not yet fully compliant with the IERS call for participation requirements. The non compliant items are the followings:

      • 3 ACs (ina, ign, gau/gsc) provide UT1 in the set of EOPs for each day while the call only expects VLBI to provides UT1,
      • lca AC applies atmospheric correction while it is requested NOT to correct for any geophysical fluid loading effects, except for tidal ocean loading.

      Concerning the last issue, LCA will provide a new SINEX series for which the weekly mean value of the atmospheric loading correction is removed.

       

      SINEX preprocessing

      The preprocessing of the SINEX solutions is realized per AC series and includes the following steps:

      • verification of DORIS station identification (dome #, mnemo)
      • rejection of stations over the whole time period (never used),
      • rejection of stations over specific periods (partially used),
      • verification of solution number and discontinuities (breaks - to be consolidated before weekly combination by analysis of all AC stations times series -),
      • when NEQ provided, inversion of free singular equations,
      • projection using minimal constraints and rejection of perturbating stations,
      • weekly comparison with ITRF2005 at epoch of each solution,
      • analysis and rejection of high residual stations.
        gop ina lca ign esa gau gsc ncl
      vs ITRF2005 t7p-I05 t7p-I05 t7p-I05 t7p-I05 t7p-I05 t7p-I05 t7p-I05  
      Internal Coherency T7p-IC T7p-IC T7p-IC T7p-IC T7p-IC T7p-IC    
      Report sum sum sum sum sum sum sum sum
      Residuals                

      (to be completed)

       

      Per week Combination

      The weekly combination results from a 7-parameter transformation calculated every week using an IDS ITRF2005 datum . This datum results from a selection of DORIS stations having the best on position (< 1 cm) and velocity (< 2 mm/yr), and included in the week solution to be processed. For each week, the steps are as follows:

      • datum generation with selection of common stations to all ACs SINEX and propagation at epoch of the solutions,
      • first CATREF combination,
      • residual analysis and station rejection (minimum number needed),
      • weighting with variance factor,
      • iteration process and final combined solution with TRF parameters.

      Note that at least 3 solutions are needed to generate a weekly combined solution. That is to say that a combination is possible over the 1997.0-2008.8 period.

      Combination results (under construction)

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      Last Updated: 02 October 2014
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      Documentation

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      About DORIS

      • Tables of data and products
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      Monitoring

      • Visualize products time series
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      • MOE statistics
      • POE statistics
       
       
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